Detection of the [C I] $λ$8727 emission line. Low-ionization structures in NGC 7009
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866909302235594752 |
|---|---|
| author | Akras, Stavros Monteiro, Hektor Walsh, Jeremy R. Konstantinou, Lydia Gonçalves, Denise R. Garcia-Rojas, Jorge Boumis, Panos Aleman, Isabel |
| author_facet | Akras, Stavros Monteiro, Hektor Walsh, Jeremy R. Konstantinou, Lydia Gonçalves, Denise R. Garcia-Rojas, Jorge Boumis, Panos Aleman, Isabel |
| contents | We report the first spatially resolved detection of the near-infrared [C I] $λ$8727 emission from the outer pair of low-ionization structures in the planetary nebula NGC 7009 from data obtained by the Multi Unit Spectroscopic Explorer integral field unit. This atomic carbon emission marks the transition zone between ionized and neutral gas, and for the first time offers direct evidence that LISs are photodominated regions. The outer LIS pair exhibits intense [C I] $λ$8727 emission, but He I $λ$8733 is absent. Conversely, the inner pair of knots shows both lines, likely due to the host nebula emission. Furthermore, the [C I] $λ$8727 line is absent in the host nebula emission, but He I $λ$8733 is present. Although the origin of the [C I] $λ$8727 line is still debated, its detection supports the scenario of photoevaporated dense molecular clumps. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_00371 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Detection of the [C I] $λ$8727 emission line. Low-ionization structures in NGC 7009 Akras, Stavros Monteiro, Hektor Walsh, Jeremy R. Konstantinou, Lydia Gonçalves, Denise R. Garcia-Rojas, Jorge Boumis, Panos Aleman, Isabel Solar and Stellar Astrophysics Astrophysics of Galaxies We report the first spatially resolved detection of the near-infrared [C I] $λ$8727 emission from the outer pair of low-ionization structures in the planetary nebula NGC 7009 from data obtained by the Multi Unit Spectroscopic Explorer integral field unit. This atomic carbon emission marks the transition zone between ionized and neutral gas, and for the first time offers direct evidence that LISs are photodominated regions. The outer LIS pair exhibits intense [C I] $λ$8727 emission, but He I $λ$8733 is absent. Conversely, the inner pair of knots shows both lines, likely due to the host nebula emission. Furthermore, the [C I] $λ$8727 line is absent in the host nebula emission, but He I $λ$8733 is present. Although the origin of the [C I] $λ$8727 line is still debated, its detection supports the scenario of photoevaporated dense molecular clumps. |
| title | Detection of the [C I] $λ$8727 emission line. Low-ionization structures in NGC 7009 |
| topic | Solar and Stellar Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2409.00371 |